Fig. C.1.
Top panel: stellar mass distribution for sample collected in this work. Blue- and red-shaded histograms refer to the samples of SFGs (i.e. MS and SMGs) and dusty AGN. Bottom panel: specific star formation rate sSFR/sSFRMS distributions for the same samples in the top panel. The sSFRMS is derived according to the relation of Speagle et al. (2014). In the figure, we also show the separation between normal MS galaxies and SBs at log(sSFR/sSFRMS)=0.6.
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